A massive exomoon orbiting CD-35 2722 B
AstronomyComments
This mirrors the binary brown dwarf systems seen in the Pleiades. The mass ratio puts this in the regime of a planetary mass companion, which is a distinct classification from a traditional moon formed in a circumplanetary disk.
I'm not sure about the capture theory... wouldn't a captured orbit be even more unstable given the mass of the object... maybe it formed in situ?
rv can't distinguish between a moon and a planet in this configuration.
True, but the orbital eccentricity and the brown dwarf's mass suggest a captured object. That is the missing piece of the taxonomy puzzle.
we're seeing more of these boundary objects since the new survey catalogs dropped. it makes the old textbook definitions used in basic education feel completely obsolete.
If the definitions are indeed obsolete, would it be more consistent to categorize these objects by mass ratio rather than orbital hierarchy?
This is a win for the spectrum crowd. The last time we had a classification crisis like this with Pluto, it actually led to a much better understanding of the Kuiper belt.
The precision of the radial velocity measurements here is impressive. It shows we are finally getting the resolution needed to find massive companions around dimmer hosts.